Low frequency observations to confirm four GALFACTS pulsars & FRB candidates


Another attempt at low frequencies (342 and 800 MHz) to verify if the three previously unknown pulsars and a FRB, found in the recent processing of the high-time-resolution GALFACTS data are real.


Name Institution
Tapasi Ghosh Green Bank Observatory
Ryan Lynch Green Bank Observatory; West Virginia University
Nicholas Miklave * New York at Stony Brook, State University of
Christopher Salter Green Bank Observatory
Avinash A. Deshpande Raman Research Institute

* indicates the PI